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20052009
most citedScaling properties of azimuthal anisotropy in Au+Au and Cu+Cu collisions at sqrt(s_NN) = 200 GeV

360 citations · 1k across the 8 of their papers we have counts for

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nucl-ex200962 cited

K/pi Fluctuations at Relativistic Energies

B. I. Abelev

We report results for fluctuations from Au+Au collisions at = 19.6, 62.4, 130, and 200 GeV using the STAR detector at the Relativistic Heavy Ion Collider. Our…

nucl-ex2008121 cited

System-size independence of directed flow at the Relativistic Heavy-Ion Collider

STAR Collaboration, B. I. Abelev

We measure directed flow () for charged particles in Au+Au and Cu+Cu collisions at 200 GeV and 62.4 GeV, as a function of pseudorapidity (), transverse mo…

nucl-ex2008102 cited

Indications of Conical Emission of Charged Hadrons at the BNL Relativistic Heavy Ion Collider

STAR Collaboration, B. I. Abelev

Three-particle azimuthal correlation measurements with a high transverse momentum trigger particle are reported for pp, d+Au, and Au+Au collisions at 200 GeV by the STAR experiment…

nucl-ex200744 cited

Source breakup dynamics in Au+Au Collisions at sqrt(s_NN)=200 GeV via three-dimensional two-pion source imaging

PHENIX Collaboration, S. Afanasiev

A three-dimensional (3D) correlation function obtained from mid-rapidity, low pT pion pairs in central Au+Au collisions at sqrt(s_NN)=200 GeV is studied. The extracted model-indepe…

nucl-ex200663 cited

System Size and Energy Dependence of Jet-Induced Hadron Pair Correlation Shapes in Cu+Cu and Au+Au Collisions at sqrt(s_NN) = 200 and 62.4 GeV

PHENIX Collaboration, A. Adare

We present azimuthal angle correlations of intermediate transverse momentum (1-4 GeV/c) hadrons from {dijets} in Cu+Cu and Au+Au collisions at sqrt(s_NN) = 62.4 and 200 GeV. The aw…

nucl-ex2006360 cited

Scaling properties of azimuthal anisotropy in Au+Au and Cu+Cu collisions at sqrt(s_NN) = 200 GeV

PHENIX Collaboration, A. Adare

Detailed differential measurements of the elliptic flow for particles produced in Au+Au and Cu+Cu collisions at sqrt(s_NN) = 200 GeV are presented. Predictions from perfect fluid h…